Magnetostratigraphy and paleomagnetism of early and middle Miocene synorogenic strata: Basement partitioning and minor block rotation in Argentine broken foreland
Magnetostratigraphic and paleomagnetic studies on early Andean synorogenic strata (Del Crestón Fm.), in the Famatina Belt (28.7°S, 67.5°W) clarify details of chronology that permit calculation of sedimentation rates within the broken foreland of west Argentina. The Del Crestón Fm represents the firs...
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2011
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| LEADER | 17239caa a22012737a 4500 | ||
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| 001 | PAPER-10893 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518204058.0 | ||
| 008 | 190411s2011 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-79951953356 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 030 | |a IJESF | ||
| 100 | 1 | |a Zambrano, O. | |
| 245 | 1 | 0 | |a Magnetostratigraphy and paleomagnetism of early and middle Miocene synorogenic strata: Basement partitioning and minor block rotation in Argentine broken foreland |
| 260 | |c 2011 | ||
| 270 | 1 | 0 | |m Rapalini, A. E.; INGEODAV, Depto. Cs. Geológicas, F.C.E.yN., Universidad de Buenos Aires and CONICET, Pabellón 2, Ciudad Universitaria, C1428EHA Buenos Aires, Argentina; email: rapalini@gl.fcen.uba.ar |
| 506 | |2 openaire |e Política editorial | ||
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| 520 | 3 | |a Magnetostratigraphic and paleomagnetic studies on early Andean synorogenic strata (Del Crestón Fm.), in the Famatina Belt (28.7°S, 67.5°W) clarify details of chronology that permit calculation of sedimentation rates within the broken foreland of west Argentina. The Del Crestón Fm represents the first record of broken foreland sedimentation within the southern Central Andean belt and the earliest retroarc volcanic rocks exposed several hundred kilometers from the trench. Twenty-five out of 49 sites collected along the succession presented a primary remanence, as determined through positive fold and reversal tests. Correlation of the local magnetic polarity section with the global polarity time scale indicates that the sedimentation of Del Crestón Fm started at ~16.7 Ma and continued until ~14.5 Ma. The youngest strata are represented by conglomerates bearing abundant Lower Paleozoic granite boulders indicating unroofing of the crystalline basement within the NW Sierras Pampeanas. This result supports the hypothesis of an early broken foreland stage at these latitudes of the Andes, with involvement of the basement in deformation and coeval retroarc volcanism, common attributes of flat-subduction regimes. A mean site paleomagnetic direction of Dec: 6.3°, Inc: -43.6° (α95: 8.0°, N = 24) confirm our earlier intrepretation that the central part of the Famatina Belt within the Sierras Pampeanas did not undergo large vertical axes rotations since the Middle Miocene. © 2010 Springer-Verlag. |l eng | |
| 536 | |a Detalles de la financiación: Universidad de Buenos Aires | ||
| 536 | |a Detalles de la financiación: Acknowledgments This study was financed through grants UBA-CyT X183 and PIP-CONICET 5783 from the Universidad de Buenos Aires and CONICET (Argentina). Further funding by FONCyT, CONICET and SECyT-UNCor to FMD and RAA is gratefully acknowledged. Mabel Mena helped us with some statistical analyses, and Rubén Somoza critically reviewed an earlier version of the manuscript. Thorough and constructive comments by T. Jordan and W. MacDonald significantly improved the original manuscript. | ||
| 593 | |a INGEODAV, Depto. Cs. Geológicas, F.C.E.yN., Universidad de Buenos Aires and CONICET, Pabellón 2, Ciudad Universitaria, C1428EHA Buenos Aires, Argentina | ||
| 593 | |a Laboratorio de Análisis de Cuencas-CICTERRA-CONICET, Cátedra de Estratigrafía y Geología Histórica, Físicas y Naturales Universidad Nacional de Córdoba, Facultad de Ciencias Exactas, Av. Velez Sarsfield 1611, 2 Piso, Of. 7, X5016GCA Córdoba, Argentina | ||
| 593 | |a Instituto Antártico Argentino, Buenos Aires, Argentina | ||
| 593 | |a IESGLO, Instituto de Sedimentología, Fundación Miguel Lillo, Miguel Lillo 251, T4000JFE San Miguel de Tucumán, Argentina | ||
| 690 | 1 | 0 | |a CENOZOIC |
| 690 | 1 | 0 | |a CENTRAL ANDES |
| 690 | 1 | 0 | |a FORELAND BASIN |
| 690 | 1 | 0 | |a MAGNETOSTRATIGRAPHY |
| 690 | 1 | 0 | |a PALEOMAGNETISM |
| 690 | 1 | 0 | |a BLOCK ROTATION |
| 690 | 1 | 0 | |a CENOZOIC |
| 690 | 1 | 0 | |a DEFORMATION MECHANISM |
| 690 | 1 | 0 | |a FORELAND BASIN |
| 690 | 1 | 0 | |a GEOCHRONOLOGY |
| 690 | 1 | 0 | |a MAGNETIC REVERSAL |
| 690 | 1 | 0 | |a MAGNETOSTRATIGRAPHY |
| 690 | 1 | 0 | |a MIOCENE |
| 690 | 1 | 0 | |a OROGENY |
| 690 | 1 | 0 | |a PALEOMAGNETISM |
| 690 | 1 | 0 | |a REMANENT MAGNETIZATION |
| 690 | 1 | 0 | |a SEDIMENTATION RATE |
| 690 | 1 | 0 | |a ANDES |
| 690 | 1 | 0 | |a SIERRAS PAMPEANAS |
| 651 | 4 | |a ARGENTINA | |
| 700 | 1 | |a Rapalini, A.E. | |
| 700 | 1 | |a Dávila, F.M. | |
| 700 | 1 | |a Astini, R.A. | |
| 700 | 1 | |a Spagnuolo, C.M. | |
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